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| | thousands of asteroids congregate in the so-called main | | thousands of asteroids congregate in the so-called main |
| | asteroid belt: a vast, doughnut-shaped ring located between | | asteroid belt: a vast, doughnut-shaped ring located between |
| − | the orbits of Mars and Jupiter from approximately 2 to 4 AU | + | the orbits of [[Mars]] and [[Jupiter]] from approximately 2 to 4 AU |
| | (186 million to 370 million miles/300 million to 600 million | | (186 million to 370 million miles/300 million to 600 million |
| | kilometers). Gaspra and Ida are main belt asteroids. | | kilometers). Gaspra and Ida are main belt asteroids. |
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| | Asteroids are thought to be primordial material | | Asteroids are thought to be primordial material |
| | prevented by Jupiter's strong gravity from accreting into a | | prevented by Jupiter's strong gravity from accreting into a |
| − | planet-sized body when the solar system was born 4.6 billion | + | planet-sized body when the [[solar system]] was born 4.6 billion |
| | years ago. It is estimated that the total mass of all | | years ago. It is estimated that the total mass of all |
| | asteroids would comprise a body approximately 930 miles | | asteroids would comprise a body approximately 930 miles |
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| | kilometers) or greater. The majority of main belt asteroids | | kilometers) or greater. The majority of main belt asteroids |
| | follow slightly elliptical, stable orbits, revolving in the | | follow slightly elliptical, stable orbits, revolving in the |
| − | same direction as the Earth and taking from three to six | + | same direction as the [[Earth]] and taking from three to six |
| | years to complete a full circuit of the Sun. | | years to complete a full circuit of the Sun. |
| | | | |
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| | Our understanding of asteroids has been derived from | | Our understanding of asteroids has been derived from |
| | three main sources: Earth-based remote sensing, data from | | three main sources: Earth-based remote sensing, data from |
| − | the Galileo flybys, and laboratory analysis of meteorites. | + | the [[Galileo Galilei|Galileo]] flybys, and laboratory analysis of meteorites. |
| | Asteroids are classified into different types according to | | Asteroids are classified into different types according to |
| | their albedo, composition derived from spectral features in | | their albedo, composition derived from spectral features in |
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| | traveling at 46,000 miles/hour (74,000 kilometers/hour) -- | | traveling at 46,000 miles/hour (74,000 kilometers/hour) -- |
| | had passed the same point in space just six hours apart. | | had passed the same point in space just six hours apart. |
| − |
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| | == External links == | | == External links == |